Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Bedregal, Alejandro G."'
Autor:
Masters, Daniel, McCarthy, Patrick, Siana, Brian, Malkan, Matthew, Mobasher, Bahram, Atek, Hakim, Henry, Alaina, Martin, Crystal L., Rafelski, Marc, Hathi, Nimish P., Scarlata, Claudia, Ross, Nathaniel R., Bunker, Andrew J., Blanc, Guillermo A., Bedregal, Alejandro G., Dominguez, Alberto, Colbert, James, Teplitz, Harry, Dressler, Alan
We present results from near-infrared spectroscopy of 26 emission-line galaxies at z ~ 2 obtained with the FIRE spectrometer on the Magellan Baade telescope. The sample was selected from the WISP survey, which uses the near-infrared grism of the Hubb
Externí odkaz:
http://arxiv.org/abs/1402.0510
Autor:
Henry, Alaina, Scarlata, Claudia, Dominguez, Alberto, Malkan, Matthew, Martin, Crystal L., Siana, Brian, Atek, Hakim, Bedregal, Alejandro G., Colbert, James W., Rafelski, Marc, Ross, Nathaniel, Teplitz, Harry, Bunker, Andrew J., Dressler, Alan, Hathi, Nimish, Masters, Daniel, McCarthy, Patrick, Straughn, Amber
We present the first robust measurement of the high redshift mass-metallicity (MZ) relation at 10^{8}< M/M_{\sun} < 10^{10}, obtained by stacking spectra of 83 emission-line galaxies with secure redshifts between 1.3 < z < 2.3. For these redshifts, i
Externí odkaz:
http://arxiv.org/abs/1309.4458
Autor:
Johnston, Evelyn J., Aragon-Salamanca, Alfonso, Merrifield, Michael R., Bedregal, Alejandro G.
Lenticular galaxies have long been thought of as evolved spirals, but the processes involved to quench the star formation are still unclear. By studying the individual star formation histories of the bulges and disks of lenticulars, it is possible to
Externí odkaz:
http://arxiv.org/abs/1309.2206
Autor:
Buitrago, Fernando, Conselice, Christopher J., Epinat, Benoit, Bedregal, Alejandro G., Grutzbauch, Ruth, Weiner, Benjamin J.
There is cumulative evidence showing that, for the most massive galaxies, the fraction of disk-like objects compared to those with spheroidal properties increases with redshift. However, this evolution is thus far based on the surface brightness stud
Externí odkaz:
http://arxiv.org/abs/1305.0268
Autor:
Buitrago, Fernando, Conselice, Christopher J., Epinat, Benoit, Bedregal, Alejandro G., Gruetzbauch, Ruth, Weiner, Benjamin J.
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2014, 439 (2), pp.1494--1521. ⟨10.1093/mnras/stu034⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 439 (2), pp.1494--1521. ⟨10.1093/mnras/stu034⟩
Monthly Notices of the Royal Astronomical Society, 2014, 439 (2), pp.1494--1521. ⟨10.1093/mnras/stu034⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 439 (2), pp.1494--1521. ⟨10.1093/mnras/stu034⟩
International audience; There is cumulative evidence showing that, for the most massive galaxies, the fraction of disc-like objects compared to those with spheroidal properties increases with redshift. However, this evolution is thus far based on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::be638e3009eb6be2833ec0241016867c
https://hal.science/hal-01434409
https://hal.science/hal-01434409
Autor:
Henry, Alaina, Scarlata, Claudia, Domínguez, Alberto, Malkan, Matthew, Martin, Crystal L, Siana, Brian, Atek, Hakim, Bedregal, Alejandro G, Colbert, James W, Rafelski, Marc, Ross, Nathaniel, Teplitz, Harry, Bunker, Andrew J, Dressler, Alan, Hathi, Nimish, Masters, Daniel, McCarthy, Patrick, Straughn, Amber
Publikováno v:
The Astrophysical Journal Letters, vol 776, iss 2
We present the first robust measurement of the high redshift mass-metallicity (MZ) relation at 108 ≲ M/M ⊙ ≲ 1010, obtained by stacking spectra of 83 emission-line galaxies with secure redshifts between 1.3 ≲ z ≲ 2.3. For these redshifts, i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::e2d43b22a41dc2bcb87cb5fe680fbe5e
https://escholarship.org/uc/item/0n89j1g7
https://escholarship.org/uc/item/0n89j1g7
Autor:
Bedregal, Alejandro G., Luis Colina, Azzollini, Ruyman, Arribas, Santiago, Alonso-Herrero, Almudena
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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By observing the local luminous infrared galaxy NGC5135 with the near-IR IFU spectrograph SINFONI (ESO-VLT), we report an approx. 600 pc (in projection) AGN outflow traced by [SiVI]1.96mum emission. This is the largest outflow traced by a coronal lin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::48da27871b2d0f09288a83c7a05a2269
http://hdl.handle.net/10261/199628
http://hdl.handle.net/10261/199628
Autor:
Arribas, Santiago, Luis Colina, Monreal-Ibero, Ana, Rodriguez-Zaurin, Javier, Alonso-Herrero, Almudena, Garcia-Marin, Macarena, Bellocchi, Enrica, Bedregal, Alejandro G., Miralles-Caballero, Daniel, Piqueras, Javier
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b8b25b2954fd44625da49c9ab1740a7b
http://hdl.handle.net/10261/199607
http://hdl.handle.net/10261/199607
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Akademický článek
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